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Deuterium and hydrogen in the local interstellar mediumDensities of neutral hydrogen and deuterium are found from observation with the Copernicus satellite of the Ly-alpha line toward two nearby stars. The hydrogen density is 0.03 + or - 0.01 per cu cm toward Alpha Aur (Capella) and 0.20 + or - 0.05 per cu cm in the direction of Alpha Cen A, values indicating that the nearby (less than 14 pc) interstellar medium is inhomogeneous and can be of low density in certain directions. The ratios of deuterium to hydrogen - 3.9 (+5.7, -1.7) by 10 to the -5th power and 0.24 (+0.12, -0.07) by 10 to the -5th power for Alpha Aur and Alpha Cen A, respectively - suggest that variations in the deuterium abundance may exist.
Document ID
19780031572
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Dupree, A. K.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Baliunas, S. L.
(Harvard College Observatory and Smithsonian Astrophysical Observatory, Center for Astrophysics, Cambridge Mass., United States)
Shipman, H. L.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 9, 2013
Publication Date
December 1, 1977
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
78A15481
Funding Number(s)
CONTRACT_GRANT: NSG-5191
CONTRACT_GRANT: NSG-5144
Distribution Limits
Public
Copyright
Other

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